Lightcurve Analysis of (12735) 1991 VV1

Details Lightcurve Analysis of (12735) 1991 VV1 Lightcurve Analysis of (12735) 1991 VV1

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007mpbu...34...83w&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Physics

Scientific paper

Observations of the main-belt asteroid (12735) 1991 VV1 were made by the authors from July through September 2006. Data from two observing sessions appeared to show deviations indicative of an eclipse or occultation by a satellite. However, extensive follow-up observations failed to provide confirming evidence and so the nature of the aberrations cannot be explained. The data did permit finding the synodic rotation period of the asteroid, that being 3.2606 ± 0.0001 hr with the amplitude of the lightcurve being 0.21 ± 0.03 mag.

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